G
G. Goldhaber
Researcher at Lawrence Berkeley National Laboratory
Publications - 16
Citations - 1959
G. Goldhaber is an academic researcher from Lawrence Berkeley National Laboratory. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 11, co-authored 16 publications receiving 1885 citations. Previous affiliations of G. Goldhaber include University of California, Berkeley.
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Journal ArticleDOI
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <z< 1.12 AND THE UNION2 COMPILATION ∗
Rahman Amanullah,Chris Lidman,David Rubin,David Rubin,Greg Aldering,Pierre Astier,Kyle Barbary,Kyle Barbary,M. S. Burns,A. Conley,Kyle S. Dawson,S. E. Deustua,Mamoru Doi,Sebastien Fabbro,L. Faccioli,L. Faccioli,H. K. Fakhouri,H. K. Fakhouri,Gastón Folatelli,A. S. Fruchter,Hisanori Furusawa,G. Garavini,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,I. M. Hook,I. M. Hook,D. A. Howell,D. A. Howell,Nobunari Kashikawa,A. G. Kim,R. A. Knop,M. Kowalski,Eric V. Linder,J. Meyers,J. Meyers,Tomoki Morokuma,S. Nobili,J. Nordin,Peter Nugent,Linda Ostman,Reynald Pain,Nino Panagia,Nino Panagia,Saul Perlmutter,Saul Perlmutter,J. Raux,Pilar Ruiz-Lapuente,A. L. Spadafora,M. Strovink,M. Strovink,Nao Suzuki,Lifan Wang,W. M. Wood-Vasey,Naoki Yasuda +55 more
TL;DR: Kowalski et al. as mentioned in this paper reported on work to increase the number of well-measured Type Ia supernovae (SNe Ia) at high redshifts.
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511
Rahman Amanullah,Chris Lidman,David Rubin,Greg Aldering,Pierre Astier,Kyle Barbary,M. S. Burns,Alex Conley,Ks S. Dawson,S. E. Deustua,Mamoru Doi,S. Fabbro,L. Faccioli,Hk K. Fakhouri,G. Folatelli,As S. Fruchter,Hisanori Furusawa,G. Garavini,G. Goldhaber,Ariel Goobar,De E. Groom,I. M. Hook,D. A. Howell,Nobunari Kashikawa,A. G. Kim,Ra A. Knop,M. Kowalski,Eric V. Linder,J. Meyers,Tomoki Morokuma,S. Nobili,J. Nordin,Pe E. Nugent,L. Ostman,R. Pain,Nino Panagia,Saul Perlmutter,J. Raux,P. Ruiz-Lapuente,A. L. Spadafora,M. Strovink,N. Suzuki,Longlu Wang,Wm M. Wood-Vasey,Naoki Yasuda,Sc Project +45 more
TL;DR: Kowalski et al. as mentioned in this paper reported on work to increase the number of well-measured Type Ia supernovae (SNe Ia) at high redshifts.
Journal ArticleDOI
Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope
David Rubin,David Rubin,R. A. Knop,Eli S. Rykoff,Eli S. Rykoff,Greg Aldering,Rahman Amanullah,K. Barbary,M. S. Burns,A. Conley,Natalia Connolly,S. E. Deustua,Vitaliy Fadeyev,H. K. Fakhouri,H. K. Fakhouri,A. S. Fruchter,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Eric Hsiao,Eric Hsiao,Eric Hsiao,Xingxing Huang,M. Kowalski,Chris Lidman,J. Meyers,J. Meyers,J. Nordin,J. Nordin,Saul Perlmutter,Saul Perlmutter,C. Saunders,C. Saunders,A. L. Spadafora,Vallery Stanishev,Nao Suzuki,Nao Suzuki,Lian-Tao Wang +38 more
TL;DR: In this paper, the authors reported the discovery of a 1.71 supernova in the GOODS-North field, which is the most distant supernova with a precision color measurement, with 92% confidence.
Journal ArticleDOI
Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study
G. Garavini,G. Garavini,Gastón Folatelli,S. Nobili,Greg Aldering,Rahman Amanullah,P. Antilogus,Pierre Astier,G. Blanc,T. J. Bronder,M. S. Burns,A. Conley,A. Conley,S. E. Deustua,Masao Doi,Sebastien Fabbro,V. Fadeyev,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,I. M. Hook,D. A. Howell,Nobunari Kashikawa,A. G. Kim,Marek Kowalski,N. Kuznetsova,Brian C. Lee,Chris Lidman,Javier Méndez,Tomoki Morokuma,Kentaro Motohara,Peter Nugent,Reynald Pain,Saul Perlmutter,Saul Perlmutter,Robert Quimby,J. Raux,Nicolas Regnault,Pilar Ruiz-Lapuente,G. Sainton,K. Schahmaneche,E. Smith,A. L. Spadafora,Vallery Stanishev,R. C. Thomas,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey,Naoki Yasuda +51 more
TL;DR: In this article, the strength of the absorption features in Type Ia supernova (SN Ia) spectra was measured and used to make a quantitative comparison between the spectra of SNe Ia at low and high redshifts.
Journal ArticleDOI
Spectra of high-redshift type Ia supernovae and a comparison with their low-redshift counterparts
I. M. Hook,D. A. Howell,Greg Aldering,Rahman Amanullah,M. S. Burns,Alex Conley,Alex Conley,S. E. Deustua,Richard S. Ellis,Sebastien Fabbro,Vitaliy Fadeyev,Gastón Folatelli,G. Garavini,G. Garavini,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,A. G. Kim,R. A. Knop,Marek Kowalski,Chris Lidman,S. Nobili,S. Nobili,Peter Nugent,Reynald Pain,C. R. Pennypacker,Saul Perlmutter,Saul Perlmutter,Pilar Ruiz-Lapuente,G. Sainton,Bradley E. Schaefer,Eric P. Smith,A. L. Spadafora,Vallery Stanishev,R. C. Thomas,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey +40 more
TL;DR: In this paper, the authors presented spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by the Supernova Cosmology Project as part of a campaign to measure cosmological parameters, and found that the dates of the spectra relative to maximum light determined from this fitting process are consistent with the dates determined from the photometric light curves, and moreover, spectral time sequences for SNe?Ia at low and high redshift are indistinguishable.